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TOI-5344 b: A Saturn-like planet orbiting a super-Solar metallicity M0 dwarf
We confirm the planetary nature of TOI-5344 b as a transiting giant exoplanet around an M0 dwarf star. TOI-5344 b was discovered with the Transiting Exoplanet Survey Satellite photometry and confirmed with ground-based photometry (the Red Buttes Observatory 0.6m telescope), radial velocity (the Habi...
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Published in: | arXiv.org 2023-11 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
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Online Access: | Get full text |
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Summary: | We confirm the planetary nature of TOI-5344 b as a transiting giant exoplanet around an M0 dwarf star. TOI-5344 b was discovered with the Transiting Exoplanet Survey Satellite photometry and confirmed with ground-based photometry (the Red Buttes Observatory 0.6m telescope), radial velocity (the Habitable-zone Planet Finder), and speckle imaging (the NN-Explore Exoplanet Stellar Speckle Imager). TOI-5344 b is a Saturn-like giant planet (\(\rho = 0.80^{+0.17}_{-0.15}\ \text{g cm}^{-3}\)) with a planetary radius of \(9.7 \pm \ 0.5 \ \text{R}_{\oplus}\) (\(0.87 \pm \ 0.04 \ \text{R}_{\text{Jup}}\)) and a planetary mass of \(135^{+17}_{-18} \text{M}_{\oplus}\) (\(0.42^{+0.05}_{-0.06} \ \text{M}_{\text{Jup}}\)). It has an orbital period of \(3.792622 \pm 0.000010\) days and an orbital eccentricity of \(0.06^{+0.07}_{-0.04}\). We measure a high metallicity for TOI-5344 of [Fe/H] = \(0.48 \pm 0.12\), where the high metallicity is consistent with expectations from formation through core accretion. We compare the metallicity of the M-dwarf hosts of giant exoplanets to that of M-dwarf hosts of non-giants (\(\lesssim 8\ \text{R}_{\oplus}\)). While the two populations appear to show different metallicity distributions, quantitative tests are prohibited by various sample caveats. |
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ISSN: | 2331-8422 |
DOI: | 10.48550/arxiv.2310.20634 |